Galactic cosmic rays on extrasolar Earth-like planets I. Cosmic ray flux
2015
(
abridgedabstract) Theoretical arguments indicate that close-in terrestial
exoplanetsmay have weak magnetic fields, especially in the case of planets more massive than Earth (
super-Earths). Planetary magnetic fields, however, constitute one of the shielding layers that protect the planet against
cosmic-rayparticles. In particular, a weak magnetic field results in a high flux of Galactic
cosmic raysthat extends to the top of the planetary atmosphere. We wish to quantify the flux of Galactic
cosmic raysto an exoplanetary atmosphere as a function of the particle energy and of the planetary magnetic moment. We numerically analyzed the propagation of Galactic
cosmic-rayparticles through planetary
magnetospheres. We evaluated the efficiency of
magnetosphericshielding as a function of the particle energy (in the range 16 MeV $\le$ E $\le$ 524 GeV) and as a function of the planetary magnetic field strength (in the range 0 ${M}_\oplus$ $\le$ {M} $\le$ 10 ${M}_\oplus$). Combined with the flux outside the planetary
magnetosphere, this gives the
cosmic-rayenergy spectrum at the top of the planetary atmosphere as a function of the planetary magnetic moment. We find that the particle flux to the planetary atmosphere can be increased by more than three orders of magnitude in the absence of a protecting magnetic field. For a weakly magnetized planet (${M}=0.05\,{M}_{\oplus}$), only particles with energies below 512 MeV are at least partially shielded. For a planet with a magnetic moment similar to Earth, this limit increases to 32 GeV, whereas for a strongly magnetized planet ($M=10.0\,{M}_{\oplus}$), partial shielding extends up to 200 GeV. We find that magnetic shielding strongly controls the number of
cosmic-rayparticles reaching the planetary atmosphere. The implications of this increased particle flux are discussed in a companion article.
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